On November 8, 1991, a major magnetic storm began with a sudden commen
cement at 0647 UT; it continued until about 1800 UT on November 9. Ass
ociated with this storm there was a great aurora which continued throu
gh November 8 and until at least 1200 UT on November 9. The first opti
cal indication of this event was the appearance of bright sun-aligned
arcs over Eureka, North West Territories (89 degrees corrected geomagn
etic latitude (CGM)), Canada from 0750 UT until about 1230 UT on Novem
ber 8. By that time, there was a gradual transformation to dominant 63
00 Angstrom emission over the central polar cap. Gradually, the major
soft electron precipitation and associated red aurora moved equatorwar
d. The aurora reached a low-latitude limit of 40 degrees CGM at 0600 U
T on November 9. The polar arcs reached 22 kR intensity (5577 Angstrom
), while the red aurora seen later at low latitudes was at least 100 k
R (6300 Angstrom). The analysis of Defense Meteorological Satellite Pr
ogram (DMSP) particle data from 83 passes during November 8 and 9 show
ed the extent and movement of precipitation from the polar region to m
idlatitudes. A comparison of this event was made with the earlier grea
t auroral event of March 13-14, 1989. While the extent in low latitude
and the duration of the two disturbances were similar, the November 8
-9 event had approximately one half of the total energy input into the
ionosphere. Its striking and unusual feature was the auroral onset an
d activity in the central polar region, a feature possibly related to
the solar wind interplanetary magnetic field orientation.